Axion-like particles with a coupling to non-Abelian gauge fields at finite temperature can
experience dissipation due to sphaleron heating. This could play an important role for warm
inflation or dynamical dark energy. We investigate to what degree the efficiency of this
non-perturbative mechanism depends on the details of the underlying particle physics model. For a
wide range of scenarios and energy scales, we find that a previously discussed suppression of
sphaleron heating by light fermions can be alleviated. As an outlook, we point out that fermionic
effects may provide a new mechanism for ending warm inflation.